Now showing items 1-4 of 4

  • Martinez, Michael N.; Napier, Kate A.; Cloonan, Aidan P.; Sukay, Ezra; Gozman, Katya; Merz, Kaiya; Khullar, Gourav; Lin, Jason J.; Matthews Acuña, Owen S.; Medina, Elisabeth; Sanchez, Jorge A.; Sisco, Emily E.; Kavin Stein, Daniel J.; Tavangar, Kiyan; González, Juan Remolina; Mahler, Guillaume; Sharon, Keren; Dahle, Håkon; Gladders, Michael D. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2023)
  • Zhang, Yunchong; Manwadkar, Viraj; Gladders, Michael D.; Khullar, Gourav; Dahle, Håkon; Napier, Kate A.; Mahler, Guillaume; Sharon, Keren; Matthews Acuña, Owen S.; Ashmead, Finian; Cerny, William; Gonzàlez, Juan Remolina; Gozman, Katya; Levine, Benjamin C.; Marohnic, Daniel; Martinez, Michael N.; Merz, Kaiya; Pan, Yue; Sanchez, Jorge A.; Sierra, Isaac; Sisco, Emily E.; Sukay, Ezra; Tavangar, Kiyan; Zaborowski, Erik (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2023)
  • Kim, Keunho J.; Bayliss, Matthew B.; Rigby, Jane R.; Gladders, Michael D.; Chisholm, John; Sharon, Keren; Dahle, Håkon; Rivera-Thorsen, Thøger Emil Juul; Florian, Michael K.; Khullar, Gourav; Mahler, Guillaume; Mainali, Ramesh; Napier, Kate A.; Navarre, Alexander; Owens, M. Riley; Roberson, Joshua (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2023)
    Abstract Extreme, young stellar populations are considered to be the primary contributor to cosmic reionization. How the Lyman continuum (LyC) escapes these galaxies remains highly elusive, and it is challenging ...
  • Sharon, Keren; Mahler, Guillaume; Rivera-Thorsen, T. Emil; Dahle, Håkon; Gladders, Michael D.; Bayliss, Matthew B.; Florian, Michael K.; Kim, Keunho J.; Khullar, Gourav; Mainali, Ramesh; Napier, Kate A.; Navarre, Alexander; Rigby, Jane R.; Remolina González, Juan David; Sharma, Soniya (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2022)
    We present a strong-lensing analysis of the cluster PSZ1 G311.65−18.48, based on Hubble Space Telescope imaging, archival VLT/MUSE spectroscopy, and Chandra X-ray data. This cool-core cluster (z = 0.443) lenses the brightest ...